Fast-rotating nearby solar-type stars - I. Spectral classification, v sin i, Li abundances and X-ray luminosities

By G. Cutispoto, L. Pastori, L. Pasquini, J. D. Medeiros, G. Tagliaferri, J. Andersen. 2002

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THE TUCANA/HOROLOGIUM, COLUMBA, AB DORADUS, AND ARGUS ASSOCIATIONS: NEW MEMBERS AND DUSTY DEBRIS DISKS (2011, methodology): “The spectrum of the star has been measured previously by Cutispoto et al. (2002), Wichmann et al. (2003), and Lopez-Santiago et al (2010).”
SPECTROSCOPIC ORBITS FOR 15 LATE-TYPE STARS (2016, background): “According to Cutispoto et al. (2002) CORAVEL velocities suggest that HD212697 is a possible single-lined spectroscopic binary.”
Young Stars Near the Sun (2004, background): “Cutispoto et al. (2002) selected 129, fast-rotating, late-F- and G-type stars brighter than V ∼ 8.6 from a CORAVEL survey.”
A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun (2010, background): “For that reason we check our star sample for pre-main sequence stars and find 236 of them either in catalogues (Chauvin et al. 2010; Ducourant et al. 2005; Hernández et al. 2005; Wichmann et al. 2005; Valenti et al. 2003; Köhler et al. 2000; Neuhäuser et al. 2000; Teixeira et al. 2000; Bertout et”